{"title":"寻找太阳发射的低质量WIMP和轴子","authors":"B. Ovchinnikov, V. Parusov","doi":"10.13189/UJPA.2016.100205","DOIUrl":null,"url":null,"abstract":"The chamber for direct detection of WIMP with mass 2 and axions, emitted from the Sun was developed. The chamber is filled with gas mixture H 2 +3ppm TMAE (1,5,10 bar), or D 2 + 3ppm TMAE. These gas fillings allow to suppress the electron background. For detecting of events is used the system GEM+pin-anode with coefficient multiplication about 10 5 . In experiment it is necessary to search the early or daily modulation effects.","PeriodicalId":23443,"journal":{"name":"Universal Journal of Physics and Application","volume":"54 6","pages":"58-59"},"PeriodicalIF":0.0000,"publicationDate":"2016-04-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"2","resultStr":"{\"title\":\"Search for Low Mass WIMP and Axions, Emitted from the Sun\",\"authors\":\"B. Ovchinnikov, V. Parusov\",\"doi\":\"10.13189/UJPA.2016.100205\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"The chamber for direct detection of WIMP with mass 2 and axions, emitted from the Sun was developed. The chamber is filled with gas mixture H 2 +3ppm TMAE (1,5,10 bar), or D 2 + 3ppm TMAE. These gas fillings allow to suppress the electron background. For detecting of events is used the system GEM+pin-anode with coefficient multiplication about 10 5 . In experiment it is necessary to search the early or daily modulation effects.\",\"PeriodicalId\":23443,\"journal\":{\"name\":\"Universal Journal of Physics and Application\",\"volume\":\"54 6\",\"pages\":\"58-59\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2016-04-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"2\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Universal Journal of Physics and Application\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.13189/UJPA.2016.100205\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Universal Journal of Physics and Application","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.13189/UJPA.2016.100205","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Search for Low Mass WIMP and Axions, Emitted from the Sun
The chamber for direct detection of WIMP with mass 2 and axions, emitted from the Sun was developed. The chamber is filled with gas mixture H 2 +3ppm TMAE (1,5,10 bar), or D 2 + 3ppm TMAE. These gas fillings allow to suppress the electron background. For detecting of events is used the system GEM+pin-anode with coefficient multiplication about 10 5 . In experiment it is necessary to search the early or daily modulation effects.
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